T
T. J. Sumner
Researcher at Imperial College London
Publications - 342
Citations - 18702
T. J. Sumner is an academic researcher from Imperial College London. The author has contributed to research in topics: Dark matter & Xenon. The author has an hindex of 62, co-authored 329 publications receiving 16405 citations. Previous affiliations of T. J. Sumner include University of Rochester & University of Florida.
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Journal ArticleDOI
First results from the LUX dark matter experiment at the Sanford Underground Research Facility
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,S. Bedikian,Ethan Bernard,A. Bernstein,Alexander Bolozdynya,A. W. Bradley,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A. A. Chiller,C. Chiller,K. Clark,T. Coffey,A. Currie,A. Curioni,Steven Dazeley,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. M. Dragowsky,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,C. E. Flores,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,Murdock Gilchriese,C. R. Hall,M. Hanhardt,S. A. Hertel,M. Horn,D. Q. Huang,M. Ihm,R. G. Jacobsen,L. Kastens,K. Kazkaz,R. Knoche,S. Kyre,R. L. Lander,N. A. Larsen,C. Lee,David Leonard,K. T. Lesko,A. Lindote,M.I. Lopes,A. Lyashenko,D.C. Malling,R. L. Mannino,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,M. Morii,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,James Nikkel,R. A. Ott,M. Pangilinan,P. D. Parker,E. K. Pease,K. Pech,P. Phelps,L. Reichhart,T. A. Shutt,C. Silva,W. Skulski,C. Sofka,V. N. Solovov,P. Sorensen,T.M. Stiegler,K. O'Sullivan,T. J. Sumner,Robert Svoboda,M. Sweany,Matthew Szydagis,D. J. Taylor,B. P. Tennyson,D. R. Tiedt,Mani Tripathi,S. Uvarov,J.R. Verbus,N. Walsh,R. C. Webb,J. T. White,D. White,M. S. Witherell,M. Wlasenko,F.L.H. Wolfs,M. Woods,Chao Zhang +101 more
TL;DR: The first WIMP search data set is reported, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data, finding that the LUX data are in disagreement with low-mass W IMP signal interpretations of the results from several recent direct detection experiments.
Journal ArticleDOI
Results from a Search for Dark Matter in the Complete LUX Exposure
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,R. Bramante,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This search yields no evidence of WIMP nuclear recoils and constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon experiment are reported.
Laser Interferometer Space Antenna
Pau Amaro-Seoane,Heather Audley,Stanislav Babak,John M. Baker,Enrico Barausse,Peter L. Bender,Emanuele Berti,Pierre Binétruy,M. Born,Daniele Bortoluzzi,Jordan Camp,Chiara Caprini,Vitor Cardoso,Monica Colpi,John Conklin,Neil J. Cornish,Curt Cutler,Karsten Danzmann,Rita Dolesi,Luigi Ferraioli,Valerio Ferroni,Ewan Fitzsimons,Jonathan R. Gair,Lluis Gesa Bote,Domenico Giardini,Ferran Gibert,Catia Grimani,Hubert Halloin,Gerhard Heinzel,Thomas Hertog,Martin Hewitson,Kelly Holley-Bockelmann,Daniel Hollington,Mauro Hueller,Henri Inchauspe,Philippe Jetzer,N. Karnesis,Christian J. Killow,Antoine Klein,Bill Klipstein,N. Korsakova,Shane L. Larson,Jeffrey Livas,Ivan Lloro,Nary Man,Davor Mance,J. Martino,Ignacio Mateos,Kirk McKenzie,Sean T. McWilliams,Cole Miller,Guido Mueller,Germano Nardini,Gijs Nelemans,Miquel Nofrarías,Antoine Petiteau,P. Pivato,Eric Plagnol,Ed Porter,J. Reiche,David J. Robertson,N. A. Robertson,Elena M. Rossi,G. Russano,Bernard F. Schutz,Alberto Sesana,David H. Shoemaker,Jacob Slutsky,Carlos F. Sopuerta,T. J. Sumner,Nicola Tamanini,Ira Thorpe,Michael Troebs,Michele Vallisneri,Alberto Vecchio,Daniele Vetrugno,Stefano Vitale,Marta Volonteri,Gudrun Wanner,H. Ward,Peter Wass,W. J. Weber,John Ziemer,Peter Zweifel +83 more
TL;DR: The LISA Consortium as mentioned in this paper proposed a 4-year mission in response to ESA's call for missions for L3, which is an all-sky monitor and will offer a wide view of a dynamic cosmos using Gravitational Waves as new and unique messengers to unveil The Gravitational Universe.
Journal ArticleDOI
Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results
Michele Armano,Heather Audley,G. Auger,J. Baird,Massimo Bassan,Pierre Binétruy,M. Born,Daniele Bortoluzzi,N. Brandt,M. Caleno,L. Carbone,Antonella Cavalleri,A. Cesarini,Giacomo Ciani,G. Congedo,A. M. Cruise,Karsten Danzmann,M. de Deus Silva,R. De Rosa,M. Diaz-Aguilo,L. Di Fiore,Ingo Diepholz,G. Dixon,Rita Dolesi,N. Dunbar,Luigi Ferraioli,Valerio Ferroni,Walter Fichter,E. D. Fitzsimons,R. Flatscher,M. Freschi,A. F. García Marín,C. García Marirrodriga,R. Gerndt,Lluis Gesa,Ferran Gibert,Domenico Giardini,R. Giusteri,F. Guzmán,Aniello Grado,Catia Grimani,A. Grynagier,J. Grzymisch,I. Harrison,Gerhard Heinzel,M. Hewitson,Daniel Hollington,D. Hoyland,Mauro Hueller,Henri Inchauspe,Oliver Jennrich,Ph. Jetzer,Ulrich Johann,B. Johlander,Nikolaos Karnesis,B. Kaune,N. Korsakova,Christian J. Killow,J. A. Lobo,Ivan Lloro,L. Liu,J. P. López-Zaragoza,R. Maarschalkerweerd,Davor Mance,V. Martín,L. Martin-Polo,J. Martino,F. Martin-Porqueras,S. Madden,Ignacio Mateos,Paul McNamara,José F. F. Mendes,L. Mendes,A. Monsky,Daniele Nicolodi,Miquel Nofrarías,S. Paczkowski,Michael Perreur-Lloyd,Antoine Petiteau,P. Pivato,Eric Plagnol,P. Prat,U. Ragnit,B. Rais,Juan Ramos-Castro,J. Reiche,D. I. Robertson,H. Rozemeijer,F. Rivas,G. Russano,J Sanjuán,P. Sarra,A. Schleicher,D. Shaul,Jacob Slutsky,Carlos F. Sopuerta,Ruggero Stanga,F. Steier,T. J. Sumner,D. Texier,James Ira Thorpe,C. Trenkel,Michael Tröbs,H. B. Tu,Daniele Vetrugno,Stefano Vitale,V Wand,Gudrun Wanner,H. Ward,C. Warren,Peter Wass,D. Wealthy,W. J. Weber,L. Wissel,A. Wittchen,A. Zambotti,C. Zanoni,Tobias Ziegler,Peter Zweifel +118 more
TL;DR: The first results of the LISA Pathfinder in-flight experiment demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density.
Journal ArticleDOI
Low-frequency gravitational-wave science with eLISA/NGO
Pau Amaro-Seoane,Sofiane Aoudia,Stanislav Babak,Pierre Binétruy,Emanuele Berti,Alejandro Bohé,Chiara Caprini,Monica Colpi,Neil J. Cornish,Karsten Danzmann,Jean-François Dufaux,Jonathan R. Gair,Oliver Jennrich,Philippe Jetzer,Antoine Klein,Ryan N. Lang,Alberto Lobo,Tyson Littenberg,Sean T. McWilliams,Gijs Nelemans,Gijs Nelemans,Antoine Petiteau,Edward K. Porter,Bernard F. Schutz,Alberto Sesana,Robin Stebbins,T. J. Sumner,Michele Vallisneri,Stefano Vitale,Marta Volonteri,H. Ward +30 more
TL;DR: The New Gravitational-Wave Observatory (NGO) as discussed by the authors, a mission under study by the European Space Agency for launch in the early 2020s, will survey the low-frequency gravitational wave sky (from 0.1 mHz to 1 Hz), detecting and characterizing a broad variety of systems and events throughout the Universe, including the coalescences of massive black holes brought together by galaxy mergers, the inspirals of stellar-mass black holes and compact stars into central galactic black holes; several millions of ultra-compact binaries, both detached and mass transferring, in